activity
20132024
most citedEnergy transfer, pressure tensor and heating of kinetic plasma

183 citations · 822 across the 28 of their papers we have counts for

collaborators

28 papers

physics.plasm-ph2024

Relativistic Alfvén turbulence at kinetic scales

Cristian Vega, Stanislav Boldyrev, Vadim Roytershteyn

In a strongly magnetized, magnetically dominated relativistic plasma, Alfvénic turbulence can extend to scales much smaller than the particle inertial scales. It leads to an energy…

physics.plasm-ph2023

Effective Viscosity, Resistivity, and Reynolds Number in Weakly Collisional Plasma Turbulence

Yan Yang, William H. Matthaeus, Sean Oughton +6

We examine dissipation and energy conversion in weakly collisional plasma turbulence, employing in situ observations from the Magnetospheric Multiscale (MMS) mission and kinetic Pa…

physics.plasm-ph2023★ 7 cited

Electron-Scale Current Sheets and Energy Dissipation in 3D Kinetic-Scale Plasma Turbulence with Low Electron Beta

Cristian Vega, Vadim Roytershteyn, Gian Luca Delzanno +1

3D kinetic-scale turbulence is studied numerically in the regime where electrons are strongly magnetized (the ratio of plasma species pressure to magnetic pressure is for…

physics.plasm-ph2023★ 10 cited

Spatial intermittency of particle distribution in relativistic plasma turbulence

Cristian Vega, Stanislav Boldyrev, Vadim Roytershteyn

Relativistic magnetically dominated turbulence is an efficient engine for particle acceleration in a collisionless plasma. Ultrarelativistic particles accelerated by interactions w…

physics.plasm-ph2022★ 10 cited

Scaling of electron heating by magnetization during reconnection and applications to dipolarization fronts and super-hot solar flares

M. Hasan Barbhuiya, Paul. A. Cassak, Michael. A. Shay +5

Electron ring velocity space distributions have previously been seen in numerical simulations of magnetic reconnection exhausts and have been suggested to be caused by the magnetiz…

physics.space-ph2022★ 43 cited

Turbulence in the outer heliosphere

Federico Fraternale, Laxman Adhikari, Horst Fichtner +9

The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with sign…